Influx of nitrogen-rich material from the outer Solar System indicated by iron nitride in Ryugu samples

Author:

Matsumoto ToruORCID,Noguchi TakaakiORCID,Miyake Akira,Igami YoheiORCID,Haruta Mitsutaka,Seto Yusuke,Miyahara MasaakiORCID,Tomioka NaotakaORCID,Saito Hikaru,Hata Satoshi,Harries DennisORCID,Takigawa AkiORCID,Nakauchi Yusuke,Tachibana ShogoORCID,Nakamura Tomoki,Matsumoto Megumi,Ishii Hope A.ORCID,Bradley John P.,Ohtaki Kenta,Dobrică ElenaORCID,Leroux Hugues,Le Guillou Corentin,Jacob DamienORCID,de la Peña Francisco,Laforet SylvainORCID,Marinova Maya,Langenhorst FalkoORCID,Beck Pierre,Phan Thi H. V.,Rebois RolandoORCID,Abreu Neyda M.,Gray Jennifer,Zega ThomasORCID,Zanetta Pierre-M.,Thompson Michelle S.,Stroud RhondaORCID,Burgess KateORCID,Cymes Brittany A.ORCID,Bridges John C.,Hicks LeonORCID,Lee Martin R.,Daly LukeORCID,Bland Phil A.,Zolensky Michael E.ORCID,Frank David R.,Martinez James,Tsuchiyama AkiraORCID,Yasutake Masahiro,Matsuno Junya,Okumura ShotaORCID,Mitsukawa Itaru,Uesugi KentaroORCID,Uesugi MasayukiORCID,Takeuchi AkihisaORCID,Sun MingqiORCID,Enju Satomi,Michikami TatsuhiroORCID,Yurimoto HisayoshiORCID,Okazaki Ryuji,Yabuta HikaruORCID,Naraoka Hiroshi,Sakamoto KanakoORCID,Yada ToruORCID,Nishimura Masahiro,Nakato Aiko,Miyazaki AkikoORCID,Yogata KasumiORCID,Abe Masanao,Okada TatsuakiORCID,Usui TomohiroORCID,Yoshikawa Makoto,Saiki Takanao,Tanaka Satoshi,Terui Fuyuto,Nakazawa SatoruORCID,Watanabe Sei-ichiroORCID,Tsuda Yuichi

Abstract

AbstractLarge amounts of nitrogen compounds, such as ammonium salts, may be stored in icy bodies and comets, but the transport of these nitrogen-bearing solids into the near-Earth region is not well understood. Here, we report the discovery of iron nitride on magnetite grains from the surface of the near-Earth C-type carbonaceous asteroid Ryugu, suggesting inorganic nitrogen fixation. Micrometeoroid impacts and solar wind irradiation may have caused the selective loss of volatile species from major iron-bearing minerals to form the metallic iron. Iron nitride is a product of nitridation of the iron metal by impacts of micrometeoroids that have higher nitrogen contents than the CI chondrites. The impactors are probably primitive materials with origins in the nitrogen-rich reservoirs in the outer Solar System. Our observation implies that the amount of nitrogen available for planetary formation and prebiotic reactions in the inner Solar System is greater than previously recognized.

Funder

MEXT | Japan Society for the Promotion of Science

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

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